Cl. Collins et Rs. Grev, RELATIVISTIC EFFECTS IN SILICON CHEMISTRY - ARE THE EXPERIMENTAL HEATS OF FORMATION OF THE SILICON ATOM AND SIH4 COMPATIBLE, The Journal of chemical physics, 108(13), 1998, pp. 5465-5468
We have investigated the effects of relativity on the atomization ener
gy of silane, SiH4, to attempt to resolve an earlier discrepancy betwe
en theory and experiment. Using a spin-free no-pair Hamiltonian that i
s based on a second-order Douglas-Kroll transformation, we find that r
elativity reduces the atomization energy of SiH4 by 0.7 kcal mol(-1):
a small change, but sufficient to bring theory and experiment into agr
eement when we include experimental uncertainties. Excitation energies
in the silicon atom, S-5(sp(3))-P-3(s(2)p(2)), and the atomic cation,
P-4(sp(2))-P-2(s(2)p), which involve a reduction in the number of s-e
lectrons, increase similar to 1.2 kcal mol(-1) when we include relativ
ity. These excitation energies show an even larger increase, about 2.5
kcal mol(-1), when we include con correlation. By contrast, the ioniz
ation potential, which involves no change in the number of s-electrons
-electron configurations s(2)p(2) in the neutral atom and s(2)p in the
cation-changes similar to 0.2 kcal mol(-1) when we include relativity
. These predictions are consistent with the notion that s-electrons ar
e the most affected by relativity, and that changes in the amount of s
-character are related, qualitatively, to differential relativistic ef
fects. (C) 1998 American Institute of Physics. [S0021-9606(98)02713-5]
.